Abstract
THE surface helium abundance of stars at the blue end of the horizontal branch in globular clusters and of halo B stars has been estimated by spectroscopists to be lower than that at the Sun's surface by factors ranging from 10 (refs. 1 and 2) to 100 (ref. 3). It is assumed that the halo B stars are the field-equivalents of horizontal branch stars, and we hereafter refer to both classes as blue horizontal branch stars.
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References
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FAULKNER, J., IBEN, I. Surface Helium Abundance in Horizontal Branch and Halo B Stars. Nature 215, 44–45 (1967). https://doi.org/10.1038/215044a0
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DOI: https://doi.org/10.1038/215044a0
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